LRD Watch DR1 · catalog object
LRDW J141903.98+524953.4
Images








3.2″ across, north up, east left, resampled from the deepest mosaic covering the object in each band; ticks mark the catalogue position. Each band is stretched on its own noise; the composite shares one flux scale, so its colour is real. No coverage in F090W.
Spectral energy distribution
- NIRCam wide
- NIRCam medium
- 2σ upper limit (S/N < 2)
At a glance
- Tier
- TENTATIVE
- Found by
- BH* channel
- Redshift
- 3.28 BH* fit
- Spectral shape
- no labelled spectrum
- F444W
- 25.81 AB S/N 69, 0.16″ aperture
- F277W − F444W
- not in the colour lane
- BH* share
- 0.82 bhs_bb4200_b8; Δχ² galaxy 3.7, dwarf 89.4
- Compactness
- growth ratio 1.652 stars 2.257
- Balmer break
- 3.41 ± 0.64 F200W/F115W, red:Hb+OIII+blue:far-uv
- Image vetting
- half-stack pass; no flags raised
- Literature
- 1 catalogue(s), 0 AGN paper(s) within 0.023″
Vetting
- Image vettingnot applicable
- Half-stack testpass
- Artifact risknone
- Neighbournone
- Extendedno
- BH* channelevidence dchi2_gal=3.7 dchi2_bd=89.4
Redshifts
Each redshift keeps its own column. Photometric redshifts of little red dots are unreliable: against spectra, about a third of AGN-template redshifts (z_agn; 31 of 95 in the last purity run) and about half of galaxy-template redshifts at z > 3 were catastrophic outliers (methods Section 8).
| Column | What it is | z | Source |
|---|---|---|---|
z_spec | Spectroscopic, DJA grade 3 | — | — |
z_vet | Adopted by vetting | 3.2834 | bhstar:bhs_bb4200_b8 |
z_phot | Photometric (P(z) peak) | — | not fitted |
z_bhs | BH* channel fit | 3.283 | bhs_bb4200_b8 |
z_agn | Colour-lane fit | — | — |
Spectral checks
- V-shape (spectrum)
- no labelled spectrum
- Star (spectrum)
- no spectrum
- V-shape (photometry)
- not measurable βUV not measured, βopt not measured at z_agn
- Line in F410M
- none 0 line-free optical band(s)
- Line-ambiguous
- no
- Settling verdict
- not evaluated
Literature
Published objects within 1″ of this position. A match is a positional recovery, not an adopted classification.
- Kokorev et al. (2024)
Photometry
Circular aperture of radius 0.16″ at each band's native resolution, background from a 0.40–0.65″ annulus, programmes combined by inverse variance. For a point source multiply by the field's aperture correction (r = 0.16″ → 0.70″). Grey rows are below S/N 2.
| Band | Instrument | Pivot (µm) | f (nJy) | σ (nJy) | AB mag | S/N | Ap. corr. |
|---|---|---|---|---|---|---|---|
| F115W | NIRCam wide | 1.154 | 14.91 | 2.68 | 28.47 | 5.6 | 1.35 |
| F150W | NIRCam wide | 1.501 | 16.50 | 3.01 | 28.36 | 5.5 | 1.34 |
| F200W | NIRCam wide | 1.989 | 50.89 | 2.73 | 27.13 | 18.7 | 1.35 |
| F277W | NIRCam wide | 2.762 | 146.53 | 2.21 | 25.98 | 66.2 | 1.44 |
| F335M | NIRCam medium | 3.362 | 132.37 | 4.22 | 26.10 | 31.4 | 1.49 |
| F356W | NIRCam wide | 3.568 | 134.42 | 2.14 | 26.08 | 62.9 | 1.51 |
| F360M | NIRCam medium | 3.624 | 145.64 | 3.89 | 25.99 | 37.4 | 1.50 |
| F410M | NIRCam medium | 4.082 | 155.08 | 3.59 | 25.92 | 43.2 | 1.53 |
| F444W | NIRCam wide | 4.404 | 171.70 | 2.50 | 25.81 | 68.8 | 1.58 |
Provenance
- Field
- EGS (CEERS pointing 3) (
miri3) - Programmes
01345, 08559behind every mosaic the field measured- Pipeline rows merged
- 1 all at one position
- Detection pass
- original
- Release build
33af9933d1cc2026-10-17T14:29:44Z
Image sources
| Band | Mosaic | Native pixel | Coverage |
|---|---|---|---|
| F115W | jw01345-o003_t023_nircam_clear-f115w_i2d.fits | 0.031″ | 1.00 |
| F150W | jw01345-o003_t023_nircam_clear-f150w_i2d.fits | 0.031″ | 1.00 |
| F200W | jw01345-o003_t023_nircam_clear-f200w_i2d.fits | 0.031″ | 1.00 |
| F277W | jw01345-o003_t023_nircam_clear-f277w_i2d.fits | 0.063″ | 1.00 |
| F356W | jw01345-o003_t023_nircam_clear-f356w_i2d.fits | 0.063″ | 1.00 |
| F410M | jw01345-o003_t023_nircam_clear-f410m_i2d.fits | 0.063″ | 1.00 |
| F444W | jw01345-o003_t023_nircam_clear-f444w_i2d.fits | 0.063″ | 1.00 |
Cite
Anderson, Jordan (2026). LRD Watch DR1: little red dot candidates from an independent search of public JWST imaging (Version DR1) [Data set]. Cerin Amroth Research. Zenodo. https://doi.org/10.5281/zenodo.23062632 Object LRDW J141903.98+524953.4.
CC BY 4.0. Please also acknowledge the JWST programmes that took the data. LRD Watch DR1 is a vetted candidate catalogue, not a complete census: it has no selection function and cannot on its own give number densities. About the release.